ORDINARY AND Z-MODE EMISSIONS FROM THE
JOVIAN POLAR-REGION
KAISER ML
DESCH MD
FARRELL WM
HESS RA
MACDOWALL RJ
PLANETARY AND SPACE SCIENCE
v.41, n.11-12, NOV-DEC, 93, p.977-985
The Ulysses Unified Radio and Plasma (URAP) experiment has detected a new
component of
Jupiter's radio spectrum in the frequency range from about 10 to 30 kHz. This
component is
emitted in the magnetoionic ordinary mode from a localized corotating source
in the northern
polar region. The source is centered at system III longitude 208-degrees,
near the meridian
containing the North magnetic dipole axis, at a distance of nearly 4R(J) from
the planet and
near the las t closed field line. The emission frequency is somewhat above
the electron plasma
frequency in the source region, but well below the electron gyrofrequency.
Accompanying this
0-mode emission at lower frequencies is intense Z-mode emission, which is
likely to play a
significant role in the generation of the 0-mode.